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<ri:Resource created="2017-04-12T08:25:18Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>DIBs in APOGEE telluric standard star spectra</title><shortName>J/A+A/600/A129</shortName><identifier>ivo://CDS.VizieR/J/A+A/600/A129</identifier><altIdentifier>doi:10.26093/cds/vizier.36000129</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Elyajouri M.</name></creator><creator><name>Lallement R.</name></creator><creator><name>Monreal-Ibero A.</name></creator><creator><name>Capitanio L.</name></creator><creator><name>Cox N.L.J.</name></creator><date role="Updated">2019-06-03T13:21:57Z</date><date role="Created">2017-04-12T08:25:18Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>interstellar-medium</subject><subject>line-intensities</subject><description>Information on the existence and properties of diffuse interstellar bands (DIBs) outside the optical domain is still limited. Additional infra-red (IR) measurements and IR-optical correlative studies are needed to constrain DIB carriers and locate various absorbers in 3D maps of the interstellar matter. We extended our study of H-band DIBs in Apache Point Observatory Galactic Evolution Experiment (APOGEE) Telluric Standard Star (TSS) spectra. We used the strong {lambda}15273 band to select the most and least absorbed targets. We used individual spectra of the former subsample to extract weaker DIBs, and we searched the two stacked series for differences that could indicate additional bands. High-resolution NARVAL and SOPHIE optical spectra for a subsample of 55 TSS targets were additionally recorded for NIR/optical correlative studies. From the TSS spectra we extract a catalog of measurements of the poorly studied {lambda}{lambda}15617, 15653, and 15673 DIBs in ~300 sightlines, we obtain a first accurate determination of their rest wavelength and constrained their intrinsic width and shape. In addition, we studied the relationship between these weak bands and the strong {lambda}15273 DIB.We provide a first or second confirmation of several other weak DIBs that have been proposed based on different instruments, and we add new constraints on their widths and locations. We finally propose two new DIB candidates. We compared the strength of the {lambda}15273 15273 absorptions with their optical counterparts {lambda}{lambda}5780, 5797, 6196, 6283, and 6614. Using the 5797-5780 ratio as a tracer of shielding against the radiation field, we showed that the {lambda}15273 DIB carrier is significantly more abundant in unshielded ({sigma}-type) clouds, and it responds even more strongly than the {lambda}5780 band carrier to the local ionizing field.</description><source format="bibcode">2017A&amp;A...600A.129E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/600/A129</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/II/149">II/149 : Diffuse Interstellar Band Measurements (Snow+ 1977)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/550/A108">J/A+A/550/A108 : DIB in VLT-FLAMES Tarantula Survey (van Loon+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/555/A25">J/A+A/555/A25 : Equivalent widths of DIBs (Puspitarini+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/72">J/ApJ/774/72 : 19 DIBs and 8 other interstellar lines (Kos+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/19">J/ApJS/225/19 : SDSS-III APOGEE spectra DIBs measurements (Elyajouri+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/463/2653">J/MNRAS/463/2653 : 8620 DIB equivalent width and extinction (Damineli+, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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DIBs</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>2MASS</name><description>2MASS name (JHHMMSSss+DDMMSSs)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>GLON</name><description>Galactic longitude</description><unit>deg</unit><ucd>pos.galactic.lon</ucd></column><column><name>GLAT</name><description>Galactic latitude</description><unit>deg</unit><ucd>pos.galactic.lat</ucd></column><column><name>EW15617</name><description>? DIB equivalent width at 15617{AA}</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EW15617</name><description>? rms uncertainty on EW15617</description><unit>0.1pm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW15653</name><description>? DIB equivalent width at 15653{AA}</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EW15653</name><description>? rms uncertainty on EW15653</description><unit>0.1pm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>EW15673</name><description>? DIB equivalent width at 15673{AA}</description><unit>0.1pm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>e_EW15673</name><description>? rms uncertainty on EW15673</description><unit>0.1pm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>lc15617</name><description>? Central wavelength of 15617 DIB (1)</description><unit>0.1nm</unit><ucd>em.wl.central</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_lc15617</name><description>? rms uncertainty on lc15617</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>lc15653</name><description>? 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